56
NMR STUDY OF THE DILUTED MAGNETIC . . .
6717
Ϫ3
relaxation times are somewhat smaller than the theoretical
ϭ␥I
͗
͘
R
of a NN cadmium nucleus, interacting with a
NN
2
ϩ
ones, but their values follow the expected changes due to the
Co at a distance RNNϭ4.3 Å in Cd1ϪxCo Se, is 11.7 kHz.
x
6
changes in R
.
With the same parameters the dipolar anisotropy of a NNN
cadmium nucleus at a distance of 6.1 Å from the Co2 ion
becomes 4.1 kHz. In the Fe alloys the dipolar anisotropies
are somewhat larger.
NNN
ϩ
IV. SUMMARY
The presence of the paramagnetic ions in the CdSe DMS
samples causes significant changes in the 1 Cd MAS NMR
spectra. Well-resolved shifted lines with short relaxation
times were observed in the Co- and Fe-based alloys. From
the temperature studies and anisotropy measurements, we
concluded that the shifts are caused by the THF interaction
between the paramagnetic ions and their NNN cadmium nu-
clei. An assignment of the 1 Cd lines of Cd0.994Co0.006Se to
the sets of NNN cations with specific bond configurations
was made by comparing experimental line intensities and
13
We measured the sideband intensities of the various cad-
mium lines in Cd0.994Co0.006Se as a function of temperature,
spinning speed, and magnetic field ͑experiments were per-
formed at 4.7 and 7.05 T͒. Spectral overlap of the sideband
patterns, poor signal-to-noise ratios and the fact that at low
temperatures the lines broaden significantly made it all diffi-
cult to perform an accurate Herzfeld-Berger analysis24 of the
MAS patterns. However, we were able to determine that the
values of the anisotropy parameter ⌬dip of all detectable
sideband patterns were in the range of 4.8Ϯ2 kHz at room
temperature and 8.0Ϯ2.5 kHz at Tϭ200 K. Because the ex-
13
relaxation times with the number of cations in these sets and
6
their T1 values calculated using their R
values. The
NNN
1
13
perimental
Cd anisotropies of the Cd1ϪxCo Se alloys are
x
strongest THF interaction occurs between a paramagnetic
2ϩ
clearly smaller than 11.7 kHz at room temperature and
smaller than 17.5 kHz at Tϭ200 K, we must conclude that
the THF-shifted lines correspond to NNN cadmium atoms.
Almost all sideband patterns had an asymmetry parameter of
about 0.1. The presence of the asymmetry indicates that the
dipolar interaction is not the only contribution to the aniso-
tropic parts of the spectra.
Co and its NNN cations at a distance 6.1 Å and with a
Ϯ60°,Ϯ60°)ϩ(Ϯ120°,Ϯ120°) configuration. The value
(
of the THF interaction is negative when the NNN cations are
2ϩ
removed from the Co ion by 8.2 Å and have a ͑120°, 180°͒
bond configuration. The smallest value is found for the all-
trans configuration. These results show the dependence of
the THF coupling constants on the type of bond conforma-
tion. It is interesting to notice that there exists some correla-
tion between the magnitudes of the THF constants and the
distances between interacting spins. In future work the de-
pendence of the THF interaction on these bond properties
should be studied theoretically by evaluating the electronic
spin polarizations in the crystal. Additionally, the values of
the electronic correlation times in the different alloys should
be evaluated in order to explain the relaxation data. The data
presented in this paper can also be used as a tool for the
determination of the incorporation of paramagnetic ions in
DMS micro- and nanoparticles.
D. Line intensities
In order to make an assignment of the spectral lines in
Figs. 1 and 2 and correlate them to the 11 sets of NNN
conformations, the relative intensities of these lines in their
fully relaxed spectrum must be compared with the number of
cadmium atoms in each set ͑see Table I͒. In addition we
expect that the values of the T1 relaxation times of these
lines are proportional to R
Eq. ͑2͒. In Table III an assignment of the lines is suggested
based on a comparison of the experimental line intensities
and the magnitudes of their spin-lattice relaxation times with
the numbers of cations in the conformational sets I–XI and
their theoretical T values, respectively. The theoretical T ’s
6
, according to the first term in
NNN
ACKNOWLEDGMENTS
1
1
The authors want to thank Professor W. Giriat for supply-
ing DMS samples and Professor W. J. M. de Jonge and Dr.
H. J. M. Swagten for stimulating discussions and advice re-
garding the analysis of our data. We wish to express our
appreciation for the stimulating discussions with Dr. D.
Zamir and his encouragement to continue the work. Part of
this work was supported by the Minerva Foundation.
were calculated using the dipolar term of Eq. ͑2͒ with
Ϫ11
6
ϭ2.5ϫ10
sec and the R
values of the assigned con-
NNN
figurations. Realizing that the signal to noise of the spectra is
rather poor and the fact that part of the spectral features
overlap, the agreement between the experimental values and
the calculated parameters is satisfactory. Most experimental
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